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After washing with water and ethanol, each for three times, the electrodes were dried by purging air.
Emphasis is placed on fluid friction, liquid flow, gas flow, corrosion, and purging air from gas lines.
The resultant rGO sheets on the electrodes, denoted as Hy-rGO, were washed with distilled water and ethanol (each for three times) and dried by purging air.
We measured their emissivity under purging air and vacuum (<0.8 mbar) conditions, at 100 °C surface temperature, using the setup described in Helbert et al. (2013) and adjusted for measuring at lower temperature, for emergence angles from 0° to 60°.
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Table 1 shows those results for emissivity difference of Millbillillie measured under purged air.
Again, we detect the narrowing of the band peaking at the CF and lowering of the continuum like for the measurements under purged air.
In this work, emissivity in vacuum was measured with the Bruker Vertex 80 V, emissivity under purged air with the Bruker IFS 88.
Figure 2 shows emissivity spectra measured under purged air for a powdered Millbillillie sample for emergence angle from 0° to 60°.
Fig. 4 Serpentinite slab emissivity measured under purged air for increasing θ; emissivity spectra of serpentinite slab sample measured under purged air at 100 °C surface temperature, for increasing emergence angle, calibrated with respect to a blackbody at the same surface temperature, measured under nadir viewing geometry.
Fig. 2 Millbillillie emissivity measured under purged air for increasing θ; emissivity spectra of meteorite Millbillillie <25 µm sample measured under purged air at 100 °C surface temperature, for increasing emergence angle, calibrated with respect to a blackbody at the same surface temperature, measured under nadir viewing geometry.
We measured the emissivity for two asteroid analogue materials (meteorite Millbillillie and a synthetic enstatite) in vacuum and under purged air, at surface temperature of 100 °C, for emergence angles of 0°, 5°, 10°, 20°, 30°, 40°, 50°, and 60°.
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